Fig. 13.
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Time delay from a bare disk as a function of the wavelength calculated with ICCF method from the artificial light curves. Model parameters: black hole mass 109 M⊙, Eddington ratio = 1.0, corona height = 5rg, inclination angle = 30 degrees, luminosity is of the order of 1045 erg s−1, and the frequency break corresponding to 75 days.
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